Low-frequency radio observations of the galaxy cluster CIZA J2242.8+5301

Some disturbed galaxy clusters host diffuse elongated radio sources, also called radio relics. It is proposed that these relics trace shock waves in the intracluster medium (ICM). Within the shock waves, generated by cluster merger events, particles are accelerated to relativistic energies, and i...

Full description

Bibliographic Details
Main Authors: Weeren, RJ van, Intema, Huib, Rottgering, H.J.A., Bruggen, M., Hoeft, M.
Format: Journal Article
Subjects:
Online Access:http://sait.oat.ts.astro.it/MSAIt820311/index.html
http://hdl.handle.net/20.500.11937/76031
_version_ 1848763608609062912
author Weeren, RJ van
Intema, Huib
Rottgering, H.J.A.
Bruggen, M.
Hoeft, M.
author_facet Weeren, RJ van
Intema, Huib
Rottgering, H.J.A.
Bruggen, M.
Hoeft, M.
author_sort Weeren, RJ van
building Curtin Institutional Repository
collection Online Access
description Some disturbed galaxy clusters host diffuse elongated radio sources, also called radio relics. It is proposed that these relics trace shock waves in the intracluster medium (ICM). Within the shock waves, generated by cluster merger events, particles are accelerated to relativistic energies, and in the presence of a magnetic field synchrotron radiation will be emitted. CIZA J2242.8+5301 is a disturbed galaxy cluster hosting complex diffuse radio emission, including a so-called double radio relic. Here we present new Giant Metrewave Radio Telescope (GMRT) radio observations of CIZA J2242.8+5301 at 325 and 150 MHz. We detect the double radio relic at 150 and 325 MHz. The very deep 150 MHz image reveals the presence of large-scale diffuse emission between the two radio relics.
first_indexed 2025-11-14T11:06:10Z
format Journal Article
id curtin-20.500.11937-76031
institution Curtin University Malaysia
institution_category Local University
last_indexed 2025-11-14T11:06:10Z
recordtype eprints
repository_type Digital Repository
spelling curtin-20.500.11937-760312019-07-23T00:46:10Z Low-frequency radio observations of the galaxy cluster CIZA J2242.8+5301 Weeren, RJ van Intema, Huib Rottgering, H.J.A. Bruggen, M. Hoeft, M. astro-ph.CO astro-ph.CO Some disturbed galaxy clusters host diffuse elongated radio sources, also called radio relics. It is proposed that these relics trace shock waves in the intracluster medium (ICM). Within the shock waves, generated by cluster merger events, particles are accelerated to relativistic energies, and in the presence of a magnetic field synchrotron radiation will be emitted. CIZA J2242.8+5301 is a disturbed galaxy cluster hosting complex diffuse radio emission, including a so-called double radio relic. Here we present new Giant Metrewave Radio Telescope (GMRT) radio observations of CIZA J2242.8+5301 at 325 and 150 MHz. We detect the double radio relic at 150 and 325 MHz. The very deep 150 MHz image reveals the presence of large-scale diffuse emission between the two radio relics. Journal Article http://hdl.handle.net/20.500.11937/76031 http://sait.oat.ts.astro.it/MSAIt820311/index.html unknown
spellingShingle astro-ph.CO
astro-ph.CO
Weeren, RJ van
Intema, Huib
Rottgering, H.J.A.
Bruggen, M.
Hoeft, M.
Low-frequency radio observations of the galaxy cluster CIZA J2242.8+5301
title Low-frequency radio observations of the galaxy cluster CIZA J2242.8+5301
title_full Low-frequency radio observations of the galaxy cluster CIZA J2242.8+5301
title_fullStr Low-frequency radio observations of the galaxy cluster CIZA J2242.8+5301
title_full_unstemmed Low-frequency radio observations of the galaxy cluster CIZA J2242.8+5301
title_short Low-frequency radio observations of the galaxy cluster CIZA J2242.8+5301
title_sort low-frequency radio observations of the galaxy cluster ciza j2242.8+5301
topic astro-ph.CO
astro-ph.CO
url http://sait.oat.ts.astro.it/MSAIt820311/index.html
http://hdl.handle.net/20.500.11937/76031